D B Sun a=5 Ranking Instructions: Rank the orbital period (from longest to shortest) of the planets. Ranking Order: Longest 1 2 4 Shortest Or, the orbital periods of the planets would all be the same. mark). (indicate with check Carefully explain your reasoning for ranking this way:

Foundations of Astronomy (MindTap Course List)
14th Edition
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Michael A. Seeds, Dana Backman
Chapter18: Origin Of The Solar System And Extrasolar Planets
Section: Chapter Questions
Problem 23RQ: Which step(s) listed in the previous question can be eliminated in models that form Jovian planets...
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How do I answer this part
Immes NeW Rollman
14px
1.5pt -
A
O X2 x2
E
Sun
B
a=5
Ranking Instructions: Rank the orbital period (from longest to shortest) of the planets.
Ranking Order: Longest 1
3
4
Shortest
Or, the orbital periods of the planets would all be the same.
mark).
(indicate with check
Carefully explain your reasoning for ranking this way:
Transcribed Image Text:Immes NeW Rollman 14px 1.5pt - A O X2 x2 E Sun B a=5 Ranking Instructions: Rank the orbital period (from longest to shortest) of the planets. Ranking Order: Longest 1 3 4 Shortest Or, the orbital periods of the planets would all be the same. mark). (indicate with check Carefully explain your reasoning for ranking this way:
Description: The figure below shows a star and five orbiting planets (A-E). Note that planets
A, B and C are in perfectly circular orbits. In contrast, planets D and E have more elliptical
orbits. Note that the closest and farthest distances for the elliptical orbits of planets D and E
happen to match the orbital distances of planets A, B, and C as shown in the figure.
E
Al
a=2
Sun
Transcribed Image Text:Description: The figure below shows a star and five orbiting planets (A-E). Note that planets A, B and C are in perfectly circular orbits. In contrast, planets D and E have more elliptical orbits. Note that the closest and farthest distances for the elliptical orbits of planets D and E happen to match the orbital distances of planets A, B, and C as shown in the figure. E Al a=2 Sun
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